A long-standing puzzle in the study of exoplanets is the formation of hot Jupiters, gas giant planets that snuggly orbit their host star. To explain their short orbital periods, theory suggests that hot Jupiters form in long orbits and then quiescently migrate through the protoplanetary disc, the flat ring of dust and debris that circles a newly fashioned star and coalesces to form the planets.
This theory was challenged when the orbital plane of hot Jupiters were discovered to be frequently misaligned with the equator of their host stars. Scientists interpreted this as evidence that hot Jupiters are the result of chaotic close encounters with other planets.
A decisive test between the two theories are systems with more than one planet: if misalignments are indeed caused by dynamical perturbations which lead to the creation of hot Jupiters, then multi-planet systems without hot Jupiters should be preferentially aligned. What new research reveals is quite different.
Using data from the NASA’s Kepler space telescope, an international research team led by Daniel Huber, a NASA Postdoctoral Program fellow at NASA’s Ames Research Center in Moffett Field, Calif., studied Kepler-56, a red giant star four times larger than the sun located at a distance of approximately 3,000 light years from Earth. By analyzing the fluctuations in brightness at different points on the surface of Kepler-56, Huber and his collaborators discovered that the star’s rotation axis is tilted by about 45 degrees to our line of sight.
“This was a surprise because we already knew about the existence of two planets transiting in front of Kepler-56. This suggested that the host star must be misaligned with the orbits of both planets,” explains Huber. “What we found is quite literally a giant misalignment in an exoplanet system.”
The culprit for the misalignment is suspected to be a third, massive companion in a long period orbit, revealed by observations obtained with the Keck telescope on Mauna Kea, Hawaii.
“Computer calculations show the outer companion may have torqued the orbital planes of the transiting planets in concert, leaving them co-planar but periodically misaligning them with the equator of the host star,” said Daniel Fabrycky, co-author and professor of astronomy at the University of Chicago.
Nearly 20 years after the discovery of the first hot Jupiter, the giant misalignment in the Kepler-56 system marks an important step towards a unified explanation for the formation of hot Jupiters.
“We now know that misalignments are not just confined to hot Jupiter systems,” said Huber. “Further observations will reveal whether the tilting mechanism in Kepler-56 could also be responsible for misalignments observed in hot Jupiter systems.”
The results are published in the Oct. 18 issue of the journal Science.
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The above story is based on materials provided by NASA.
Note: Materials may be edited for content and length. For further information, please contact the source cited above.
D. Huber, J. A. Carter, M. Barbieri, A. Miglio, K. M. Deck, D. C. Fabrycky, B. T. Montet, L. A. Buchhave, W. J. Chaplin, S. Hekker, J. Montalban, R. Sanchis-Ojeda, S. Basu, T. R. Bedding, T. L. Campante, J. Christensen-Dalsgaard, Y. P. Elsworth, D. Stello, T. Arentoft, E. B. Ford, R. L. Gilliland, R. Handberg, A. W. Howard, H. Isaacson, J. A. Johnson, C. Karoff, S. D. Kawaler, H. Kjeldsen, D. W. Latham, M. N. Lund, M. Lundkvist, G. W. Marcy, T. S. Metcalfe, V. Silva Aguirre, J. N. Winn. Stellar Spin-Orbit Misalignment in a Multiplanet System. Science, 2013; 342 (6156): 331 DOI: 10.1126/science.1242066
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